Superfluid Helium-3: Universal Concepts for Condensed Matter and the Big Bang

Transcription

1 Center for Electronic Correlations and Magnetism University of Augsburg Superfluid Helium-3: Universal Concepts for Condensed Matter and the Big Bang Dieter Vollhardt Physikalisches Kolloquium, Universität Heidelberg; December 8, 2017

2 Helium Two stable Helium isotopes: 4 He, 3 He 4 He: air, oil wells,... Janssen/Lockyer/Secci (1868) He air He He air Ramsay (1895) Cleveit (UO 2 ) 3 He: Li + n H + α He 2 Research on macroscopic samples of 3 He only since He: Coolant, Welding, Balloons 3 He: - Contrast agent in medicine - Neutron detectors - 3 He- 4 He dilution refrigerators (quantum computers!)

3 Helium Atoms: spherical, hard core diameter 2.5 Å Interaction: hard sphere repulsion van der Waals dipole/multipole attraction Boiling point: 4.2 K, 4 He Kamerlingh Onnes (1908) 3.2 K, 3 He Sydoriak et al. (1949) Dense, simple liquids { isotropic short-range interactions extremely pure

4 Helium 40 P (bar) [10 bar = 1 MPa] solid superfluid superfluid? 3 He 4 He normal fluid λ-line T(K) vapor T 0, P < 30 bar: Helium remains liquid λ kt B T 0 quantum phenomena on a macroscopic scale

5 Helium 4 He 3 He Electron shell: 2 e -, S = 0 Nucleus: p n n p n p p Atom(!) is a S = 0 Boson S = 1 2 Fermion Quantum liquids Phase transition T λ = 2.2 K Bose-Einstein condensation superfluid with frictionless flow T c =???

6 Interacting Fermions (Fermi liquid): Ground state k z Landau (1956/57) E F : Fermi surface k y k x Fermi sphere + 2 non-interacting fermions

7 Interacting Fermions (Fermi liquid): Ground state Arbitrarily weak attraction k instability k z Cooper (1956) E = 2 ε exp( 2 / N(0) V ) c ε c <<E F L E F : Fermi surface k y k x k Cooper pair Universal property of Fermi systems

8 Cooper pair ( k, α; k, β) k,α Ψ L= 0,2,4,... = ψ () r S=0 (singlet) ξ 0 Antisymmetry k, β Ψ = r + L= 1,3,5,... ψ () + ψ () r ψ () - r S=1 (triplet) L = 0 ( s-wave ): isotropic pair wave function L > 0 ( p,d,f, -wave ): anisotropic pair wave function 3 He: Strongly repulsive interaction L > 0 expected

9 BCS theory Bardeen, Cooper, Schrieffer (1957) Generalization to macroscopically many Cooper pairs Pair condensate Energy gap Δ(T) here: L=0 (s-wave) ε c <<E F E F transition temperature T = 1.13 ε exp( 1/ N( 0) V ) c c L ε c, V L : Magnitude? Origin? T c? Thanksgiving 1971: Transition in 3 He at T c = K Osheroff, Richardson, Lee (1972) Osheroff, Gully, Richardson, Lee (1972)

10 The Nobel Prize in Physics 1996 "for their discovery of superfluidity in helium-3" David M. Lee Cornell (USA) Douglas D. Osheroff Stanford (USA) Robert C. Richardson Cornell (USA)

11 Phase diagram of Helium-3 P-T phase diagram Dense, simple liquid { isotropic short-range interactions extremely pure nuclear spin S=1/2 ordered spins disordered spins Fermi liquid Solid (bcc)

12 Phase diagram of Helium-3 P-T phase diagram Dense, simple liquid { isotropic short-range interactions extremely pure nuclear spin S=1/2 viscosity zero high viscosity (machine oil)

13 Phase diagram of Helium-3 P-T-H phase diagram Millikelvin Cryostat WMI Garching Very (ultra) low temperatures : T << T boiling ~ 3 K and << T backgr. rad. ~ 3 K

14 Superfluid phases of 3 He Experiment: Osheroff, Richardson, Lee, Wheatley,... Theory: Leggett, Wölfle, Mermin, L=1, S=1 ( p-wave, spin-triplet ) in all 3 phases anisotropy directions in every 3 He Cooper pair ˆd ˆl orbital part spin part Attraction due to spin fluctuations S=1 Anderson, Brinkman (1973)

15 and a mystery! NMR experiment on nuclear spins I= 1 2 Osheroff et al. (1972) ω ω ω L T ( ) 3mT?! ω L ω Larmor frequency: L = γ H superfluid Shift of ω L T C,A normal T spin-nonconserving interactions nuclear dipole interaction g D 10 7 K TC Origin of frequency shift?! Leggett (1973)

16 The superfluid phases of 3 He

17 B-phase All spin states, +, occur equally ( k) = 0 Balian, Werthamer (1963) Vdovin (1963) energy gap Fermi sphere (pseudo-) isotropic state s-wave superconductor Weak-coupling theory: stable for all T<T c

18 A-phase Spin states, occur equally strong gap anisotropy ( k ˆ ) = sin( kl ˆ, ˆ ) Anderson, Morel (1961) 0 ˆl Cooper pair orbital angular momentum energy gap Fermi sphere Energy gap with point nodes axial (chiral) state helped to understand heavy fermion superconductors (CeCu 2 Si 2, UPt 3, ) high-t c (cuprate) superconductors Strong-coupling effect

19 3 He-A: Spectrum near nodes ˆl ˆl ^ l The Universe in a Helium Droplet, Volovik (2003) E k Energy Egap k Excitations Fermi sea = Vacuum k ( ) 2 E = v k k sin ( ˆˆ F + kl, ) e k F = 1 kˆ kˆ + lˆ lˆ chirality up chirality down ij = g pp i j Fermi point: spectral flow of fermionic charge Lorentz invariance ij 2 g = v Fll i j+ ( δij ll i j) kf 2 Chiral (Adler) anomaly in 3 He-A observed Bevan et al. (1997)

20 A 1 -phase in finite magnetic field Only spin state Long-range ordered magnetic liquid

21 Broken Symmetries & Long-Range Order

22 Broken Symmetries & Long-Range Order Normal 3 He 3 He-A, 3 He-B: 2 nd order phase transition T<T c : higher order, lower symmetry of ground state I. Ferromagnet Average magnetization: T>T c T<T c M = 0 M 0 Order parameter Symmetry group: SO(3) U(1) SO(3) T<T C : SO(3) rotation symmetry in spin space spontaneously broken

23 Broken Symmetries & Long-Range Order Normal 3 He 3 He-A, 3 He-B: 2 nd order phase transition T<T c : higher order, lower symmetry of ground state II. Liquid crystal T>T c T<T c Symmetry group: SO(3) U(1) SO(3) T<T C : SO(3) rotation symmetry in real space spontaneously broken

24 Broken Symmetries & Long-Range Order Normal 3 He 3 He-A, 3 He-B: 2 nd order phase transition T<T c : higher order, lower symmetry of ground state III. Conventional superconductor T>T c T<T c Pair amplitude c c 0 i e φ k k complex order parameter = iϕ Gauge transf. ck σ ck σe : gauge invariant not gauge invariant Symmetry group U(1)

25 Broken Symmetries & Long-Range Order Normal 3 He 3 He-A, 3 He-B: 2 nd order phase transition T<T c : higher order, lower symmetry of ground state III. Conventional superconductor T>T c T<T c T<T C : U(1) gauge symmetry spontaneously broken

26 Broken symmetries in superfluid 3 He L=1, S=1 in all 3 phases Cooper pair: ˆd ˆl orbital part spin part Quantum coherence in { phase (complex order parameter) anisotropy direction in real space anisotropy direction in spin space Superfluid, liquid crystal magnet Characterized by 2 (2L + 1) (2S + 1) = 18 real numbers 3x3 order parameter matrix A iμ SO(3) S SO(3) L U(1) φ symmetry spontaneously broken SU(2) L SU(2) R U(1) Y for electroweak interactions Leggett (1975) Pati, Salam (1974)

27 Broken symmetries in superfluid 3 He Mineev (1980) Bruder, Vollhardt(1986) 3He-B SO(3) S SO(3) L U(1) φ symmetry broken SO(3) S+L _ Unconventional" pairing Spontaneously broken spin-orbit symmetry Leggett (1972) Cooper pairs Fixed relative orientation

28 Broken symmetries in superfluid 3 He Mineev (1980) Bruder, Vollhardt(1986) 3He-B SO(3) S SO(3) L U(1) φ symmetry broken SO(3) S+L _ Unconventional" pairing Relation to particle physics Isodoublet u d, u d L R chiral invariance Global symmetry SU(2) L SU(2) R qq condensation ( Cooper pair ) SU(2) L+R Goldstone excitations (bosons) 3 pions

29 Broken symmetries in superfluid 3 He Mineev (1980) Bruder, Vollhardt(1986) 3He-A SO(3) S SO(3) L U(1) φ symmetry broken U(1) Sz U(1) Lz - φ Unconventional" pairing ˆl Cooper pairs Fixed absolute orientation

30 solves the NMR mystery

31 Superfluid 3 He - a quantum amplifier Cooper pairs in 3 He-A Fixed absolute orientation What fixes the relative orientation of? ˆ, d ˆl Interaction of nuclear dipoles ( spin-orbit coupling ) : Dipole-dipole coupling of 3 He nuclei: g D 10 7 K TC Unimportant?!

32 Superfluid 3 He - a quantum amplifier Cooper pairs in 3 He-A Fixed absolute orientation But: Long-range order in d ˆ, ˆl 7 g 10 K : tiny, but lifts degeneracy of relative orientation D d ˆ, ˆl quantum coherence locked in all Cooper pairs at a fixed angle NMR frequency increases: 2 2 ω = ( γ H ) + g 2 D ( T ) Leggett (1973) Nuclear dipole interaction is macroscopically measurable

33 The Nobel Prize in Physics 2003 "for pioneering contributions to the theory of superconductors and superfluids" Alexei A. Abrikosov USA and Russia Vitaly L. Ginzburg Russia Anthony J. Leggett UK and USA

34 Order-parameter textures and topological defects

35 Order-parameter textures in 3 He-A Orientation of the macroscopic anisotropy directions d ˆ, ˆl : 1) Walls ˆl or 2) Magnetic field ˆd Chirality exp. confirmed: Walmsley, Golov (2012) Textures in d ˆ, ˆl liquid crystals

36 Order-parameter textures and topological defects in 3 He-A D=2: domain walls (solitons) in ˆd or ˆl because of ˆl ˆl Z 2 symmetry Cannot be removed by local operation topological defect Single domain wall ˆd ˆl ˆd Domain wall lattice

37 Order-parameter textures and topological defects in 3 He-A D=1: Vortices Vortex formation by rotation e.g., Mermin-Ho vortex (non-singular) Thin film of 3 He-A Skyrmion vortex Volovik (2003), Sauls (2013)

38 Order-parameter textures and topological defects in 3 He-A D=0: Monopoles Boojum in ˆl -texture of 3 He-A Defect formation by rotation geometric constraints rapid crossing through symmetry breaking phase transition

39 Big bang simulation in the low-temperature lab

40 Universality in symmetry-breaking phase transitions High symmetry, short-range order T>T c Spins: paramagnetic Helium: normal liquid Universe: Unified forces and fields T=T c Phase transition Broken symmetry, long-range order ferromagnetic superfluid elementary particles, fundamental interactions Defects: domain walls vortices, etc. cosmic strings, etc. Kibble (1976) T<T c nucleation of galaxies?

41 Rapid thermal quench through 2 nd order phase transition Bäuerle et al. (1996) 1. Local temperature T T c 3. Expansion + rapid cooling through T c Defects overlap 2. Nucleation of independently ordered regions Clustering of ordered regions Defects form 4. Vortex tangle Estimate of density of defects: Zurek (1985) Kibble-Zurek mechanism of defect formation: How to test?

42 Big-bang simulation in the low-temperature laboratory Grenoble: Bäuerle et al. (1996), Helsinki: Ruutu et al. (1996) 3 He-B NMR Measured vortex-tangle density: Quantitative support for Kibble-Zurek mechanism

43 Current research on superfluid 3 He 3 He in 98% open silica aerogel 1. Influence of disorder on superfluidity 3 He Halperin et al. (2008) SiO 2 2. Quantum Turbulence No friction only vortex tangle Origin of decay of pure superfluid turbulence? Test systems: 4 He-II, 3 He-B Vortex tangle Tsubota (2008) 3. Majorana fermions (e.g., zero-energy Andreev bound states at surfaces in 3 He-B) Majorana cone for 3 He-B in a thick slab Tsutsumi, Ichioka, Machida (2011)

44 The Superfluid Phases of Helium 3 D. Vollhardt and P. Wölfle (Taylor & Francis, 1990), 656 pages Reprinted by Dover Publications (2013)

45 Conclusion Superfluid Helium-3: Anisotropic superfluid (p-wave, spin-triplet pairing) - Cooper pairs with internal structure - 3 different bulk phases with many novel properties Large symmetry-group broken - Close connections with high energy physics - Zoo of topological defects